• Journal of the Optical Society of Korea
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• 제19권5호
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• pp.494-502
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• 2015

This paper introduces methods to measure vibration using a fringe pattern. These methods use variations of a fringe pattern in reflective monochromatic interferometry, without additional components. With the proposed methods we measured the vibrations of four waveform with amplitude 100 nm. When the vibrational amplitude is greater than a quarter wavelength of the light employed, however, the measured results are distorted due to ambiguity. Thus we propose advanced methods to solve this problem, and also measure the vibrations of two waveformswith an amplitude of $1{\mu}m$. To verify the performance of the proposed methods, we compare the results to those from an accelerometer. Multifrequency vibrations of 1, 5, 10, and 20 Hz are measured by both techniques, and the results compared in the frequency domain.

• ETRI Journal
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• 제9권3호
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• pp.74-85
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• 1987

본 논문은 PARCOR형 DTMF신호 수신방식을 이용하는 대역내 신호방식에 관하여 논한다. PARCOR 계수의 움직임에 관한 관찰 및 분석을 통하여 제안된 수신기의 성능평가, 즉 음성면역, 잡음면역 및 누화에 대한 면역 성능을 평가하고 이에 따른 수신 알고리즘 설계의 예를 제시한다.

• 대한전자공학회:학술대회논문집
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• 대한전자공학회 2000년도 ITC-CSCC -1
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• pp.105-108
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• 2000

The economical detection of dual-tone multifrequency(DTMF) signals is an important factor when developing cost-effective telecommunication equipment. Each channel has independently a DTMF receiver, and I t informs the detected signal to processors. This paper analyze the power spectra and evaluate the performance of DTMF receiver by using tile quick Fourier transform(QFT) algorithm. As experimental results, it show the improved performance to the DTMF receivers and reduce memory waste and process the real-time.

• 천문학회보
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• 제36권1호
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• pp.50.1-50.1
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• 2011

We report the results of the monitoring of a flaring gamma-ray blazar, 3C454.3 in total flux density at 22 and 43GHz and in polarization at 22GHz with KVN Ulsan 21-m radio telescope every 3-4 days from 19 November 2010 to 31 January 2011. After an extraordinary 5-day gamma-ray outburst in November 2010, the radio total flux density at 22/43GHz and the linear polarization at 22GHz has been decreased with a variation of a short time scale. In this paper, we also discuss a spectral change of 3C454.3 at 22 and 43GHz after the extraordinary gamma-ray outburst.

• 대한의용생체공학회:학술대회논문집
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• 대한의용생체공학회 1996년도 추계학술대회
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• pp.185-188
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• 1996

Noninvasive multifrequency microwave radiometry using coaxial waveguide antenna has been investigated for a homogeneous and four layer human body model. The coupling between coaxial waveguide antenna and a. biological object is analyzed by use of the FDTD method to obtain the absorbed power patterns in the media. The object studied in this paper is a homogeneous and four-layered lossy medium. The specific absorption rates(SAR) distribution is calculated in each region by use of the steady-state response in FDTD method.

• 비파괴검사학회지
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• 제30권2호
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• pp.155-161
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• 2010

전자기유도(electromagnetic induction) 현상을 이용한 비파괴진단기법으로 최근까지 와전류탐상기법, 교류장측정기법, 자속누설검사기법, 그리고 원격장검사기법 등이 개발되어 활용되고 있었다. 이 기법중 와전류탐상기법은 오늘날 발전설비, 화학, 조선 및 군수설비 등의 열교환기 전열관 비파괴검사에 널리 적용되고 있다. 와전류탐상검사 시스템의 구성은 기능별로 와전류신호 합성 모듈, 아날로그 모듈, 디지털 신호처리를 위한 아날로그-디지털 변환 모듈, 전원공급장치 및 신호취득 평가 프로그램 등으로 구성되며, 본 연구에서는 다중채널방식의 와전류탐상검사 장치(하드웨어) 개발에 필요한 구성 요소중 1차적으로 와전류신호 합성 모듈, 아날로그 모듈을 설계 개발하였다. 본 연구에서 개발한 와전류탐상검사 장치의 특정은 주파수영역 및 시간영역 다중화 방식에 의한 최대 4개 주파수의 동시 적용이 가능한 다중채널장치이다. 와전류신호 합성 모듈, 아날로그 모듈을 구성하는 각 회로에서 와전류신호 발생, 변조, 전처리, 변조 및 신호 디스플레이를 위한 신호가 적절하게 처리되어 최종적으로 와전류신호 평가에 필수적인 리사쥬신호가 임피던스 평면 내에 디스플레이 되는 것을 확인하였다.

• 천문학회지
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• 제36권spc1호
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• pp.29-36
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• 2003

Quiescent solar radiation, at microwave spectral regime, is dominated by gyroresonant and thermal Bremsstrahlung radiations from hot electrons residing in solar active region corona. These radiations are known to provide excellent diagnostics on the coronal temperature, density, and magnetic field, provided that spatially resolved spectra are available from observations. In this paper we present an imaging spectroscopy implemented for a bipolar active region, AR 7912, using the multifrequency interferometric data from the Owens Valley Solar Array (OVSA), as processed with a new imaging technique, so-called Spatio-Spectral Maximum Entropy Method (SSMEM). From the microwave maps at 26 frequencies in the range of 1.2-12.4 GHz at both right- and left-circular polarizations, we construct spatially resolved brightness spectra in every reconstructed pixel of about 2 arcsec interval. These spectra allowed us to determine 2-D distribution of electron temperature, magnetic field of coronal base, and emission measure at the coronal base above the active region. We briefly compare the present result with existing studies of the coronal active regions.

• 대한물리치료과학회지
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• 제10권2호
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• pp.137-144
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• 2003

The purpose of this study was to investigate the difference of body composition of the elderly according to the age. This study consisted of elder male(n=48) and elder female(n=58). The average age of male elder and female elder was 73.81, 73.05 years. The data were analyzed with t-test, using SPSSWIN 10.1 program. Body composition was measured using Inbody 3.0(seoul, korea) of segmental multifrequency impedance analyzer technique. The result of this study were the following : 1. The difference of body composition according to the age 1) The MV(Muscle Volume)of male elder was significant difference among group(p<.05). The MV of female elder was very significant difference among group(p<.01). 2) The %FAT of male elder and female elder was no significant difference among group. 3) The FFM(Free Fat Mass)of male elder was significant difference among group(p<.05). The FFM of female elder was very significant difference among group(p<.01). 4) The TBW(Total Body Water)of male elder was significant difference among group(p<.05) The TBW of female elder was very significant difference among group(p<.01). 5) The WHR(Waist to Hip Ratio)of male elder was significant difference among group(p<.05). The WHR of female elder was very significant difference among group(p<.01).

• 천문학회보
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• 제39권2호
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• pp.60.1-60.1
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• 2014

In the center of an Active Galactic Nuclei(AGN) is a supermassive black hole which accretes matter from its surroundings. The radio-loud AGN launch two relativistic jets perpendicular to the accretion disk which terminates into radio lobes located up to megaparsec away. Blazars form a small subset of radio-loud AGNs with one of two relativistic jets pointing toward the observer's line of sight. Many blazars often show flares at different frequencies. And these flares at different frequencies are known that they often correlate with each other. In 2013 December, there was a gamma-ray flare in 3C 279, one of the brightest blazars, Dec 2013. So we want to reveal that whether this flare correlates with radio flare or not, and where the flare originate. With polarization observation at radio frequencies, we can study the physical properties of the magnetic field in the innermost regions of the relativistic jets. Therefore, we have conducted polarization monitoring of this source from Dec. 2013 to Jun. 2014 with KVN(Korea VLBI Network) radio telescopes at 22, 43 and 86GHz. Here we present the initial results of the monitoring of 3C 279. We prospect that we can reveal the origin of this gamma-ray flare by comparing with our radio data.

• 대한전자공학회논문지
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• 제20권3호
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• pp.29-32
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• 1983

본 논문에서는 ROM table look-up 방법에 의한 주파수 발생원리 및 이를 이용하여 전자교환국간의 신호방식에 사용되는 MF(multi-frequency) 디지탈 송신기의 설계에 관하여 고찰하였다. 그리고 실제로 MF 디지탈 송신기를 구성한 후 실험을 통해 신호의 규격을 충분히 만족시킴을 알 수 있었고, 이러한 근본적인 원리는 음성대역내의 주파수에 의한 신호방식에 적용이 가능함을 알 수 있으며 또한 전자교환기 국간 신호방식으로 사용되는 R2-MFC 신호 장비에도 이같은 원리를 적용하여 구성할 수 있음을 알 수 있다.